OPTICAL-INFRARED AND HIGH-ENERGY ASTRONOMY COLLABORATION AT HIROSHIMA ASTROPHYSICAL SCIENCE CENTER | Zendy

Makoto Uemura | Zendy; M. Yoshida | Zendy; Koji S. Kawabata | Zendy; Tsunefumi Mizuno | Zendy; Yasuyuki Tanaka | Zendy; Hiroshi Akitaya | Zendy; Yousuke Utsumi | Zendy; Yuki Moritani | Zendy; R. Itoh | Zendy; Y. Fukazawa | Zendy; H. Takahashi | Zendy; M. Ohno | Zendy; Takahiro Ui | Zendy; K. Takaki | Zendy; N. Ebisuda | Zendy; Kenji Kawaguchi | Zendy; KENSYO MORI | Zendy; Y. Ohashi | Zendy; Yuka Kanda | Zendy; Miho Kawabata | Zendy; Koji Takata | Zendy; Tatsuya Nakaoka | Zendy

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OPTICAL-INFRARED AND HIGH-ENERGY ASTRONOMY COLLABORATION AT HIROSHIMA ASTROPHYSICAL SCIENCE CENTER

Author(s) -

Makoto Uemura,

M. Yoshida,

Koji S. Kawabata,

Tsunefumi Mizuno,

Yasuyuki Tanaka,

Hiroshi Akitaya,

Yousuke Utsumi,

Yuki Moritani,

R. Itoh,

Y. Fukazawa,

H. Takahashi,

M. Ohno,

Takahiro Ui,

K. Takaki,

N. Ebisuda,

Kenji Kawaguchi,

KENSYO MORI,

Y. Ohashi,

Yuka Kanda,

Miho Kawabata,

Koji Takata,

Tatsuya Nakaoka

Publication year - 2015

Publication title -

publications of the korean astronomical society

Language(s) - English

Resource type - Journals

eISSN - 2287-6936

pISSN - 1225-1534

DOI - 10.5303/pkas.2015.30.2.679

Subject(s) - infrared , physics , astronomy , center (category theory) , high energy , high energy astronomy , infrared astronomy , astrophysics , engineering physics , chemistry , cosmic ray , crystallography

The Hiroshima Astrophysical Science Center (HASC) was founded in 2004 at Hiroshima University, Japan. The main mission of this institute is the observational study of various transient objects including gamma-ray bursts, supernovae, novae, cataclysmic variables, and active galactic nuclei by means of multi-wavelength observations. HASC consists of three divisions; the optical-infrared astronomy division, high-energy astronomy division, and theoretical astronomy division. HASC is operating the 1.5m optical-infrared telescope Kanata, which is dedicated to follow-up and monitoring observations of transient objects. The high-energy division is the key operation center for the Fermi gamma-ray space telescope. HASC and the high-energy astronomy group in the department of physical science at Hiroshima University are closely collaborating with each other to promote multi-wavelength time-domain astronomy. We report the recent activities of HASC and some science topics pursued by this multi-wavelength collaboration.

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